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- W2021195590 abstract "X-ray emission is modeled and x-ray intensities are predicted for Venus and Mars. Two emission mechanisms are studied: (1) elastic scattering of solar x-rays by atmospheric neutrals, (2) absorption of solar x-rays in either the carbon or oxygen K-shells followed by fluorescent emission of x-rays. The carbon and oxygen atoms reside in the carbon dioxide molecules. We predict total soft x-ray intensities of approximately 0.67 R for Venus and 0.15 R for Mars, corresponding to total soft x-ray luminosities of about 35 MW and 2.5 MW, respectively. These luminosities exceed the x-ray luminosities expected from the solar wind charge exchange mechanism." @default.
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- W2021195590 date "2001-08-01" @default.
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- W2021195590 title "X-ray emission from scattering and fluorescence of solar X-rays at Venus and Mars" @default.
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- W2021195590 doi "https://doi.org/10.1029/2001gl013021" @default.
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